Tomimatsu-Sato solutions describe cosmic strings interacting with gravitational waves

Details Tomimatsu-Sato solutions describe cosmic strings interacting with gravitational waves Tomimatsu-Sato solutions describe cosmic strings interacting with gravitational waves

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvd..41.2512p&link_type=abstract

Physical Review D (Particles and Fields), Volume 41, Issue 8, 15 April 1990, pp.2512-2518

Physics

10

Exact Solutions, Particle-Theory And Field-Theory Models Of The Early Universe

Scientific paper

We demonstrate that the proper place of the Tomimatsu-Sato solutions is in the description of cylindrically symmetric spacetimes, as opposed to stationary axisymmetric spacetimes. More particularly, we consider a version of the δ~=2 Tomimatsu-Sato solutions, obtained from the standard Tomimatsu-Sato solutions by an analytic continuation, that describe a cylindrically symmetric spacetime. It admits a regular axis, is asymptotically flat, and is smooth everywhere but the axis where it exhibits a conical, but not a curvature, singularity. The spacetime describes a beam-like-shaped pulse of gravitational radiation scattered by a cosmic string.

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